On the different flavours of Lense-Thirring precession around accreting stellar mass black holes
S.E. Motta, A. Franchini, G. Lodato, G. Mastroserio

TL;DR
This paper compares test particle and global precession models for Type-C QPOs in X-ray binaries, showing their relation, implications for black hole spin measurements, and conditions for coherent precession.
Contribution
It demonstrates that the test particle model is a limiting case of the global model and clarifies conditions for stable, coherent precession in accretion flows.
Findings
Test particle model is a limit of the global model.
Global model explains observed QPO frequencies without flow truncation.
Narrow, radially confined flows are necessary for rigid precession.
Abstract
Type-C QPOs in X-ray binaries have been often interpreted as a consequence of relativistic Lense-Thirring precession around a spinning black hole and they potentially offer a way to measure black hole spins and masses. The connection between relativistic precession and the resulting QPO has been made either in terms of a simplified model involving a single test particle producing the QPO, or in terms of a global model where a geometrically thick accretion flow precesses coherently as a rigid body. In this paper, we analyse similarities and differences between these two models, sometimes considered as in opposition to each other. We demonstrate that the former is the limiting case of the latter when the radial extent of the precessing flow is very small, and that solid lower limits to the black hole spin can be obtained by considering the test particle model alone. We also show that the…
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